Is it possible that the question models an s-orbital (where the boundary surface is a neat sphere)? From my understanding, the probability |ψ|^2 would be constant all over the surface ...
Is this condition valid for other orbital shapes? I don't think so.
|ψ|² is proportional to the electron density, so a surface of constant |ψ|² is also a surface of constant electron density. And this is what we normally take to mean the shape of the orbital.
So for all orbitals the shapes of the orbitals you see drawn in books are surfaces of constant |ψ|².
A surface of constant |ψ|² is also a surface of constant |ψ|, but it isn't clear what the question means by asking if the surfaces are different.
@JohnRennie yes i looked into it for a few more hours, the air is turbulent close to the fireplace, which causes imbalance and if the motors can't generate enough RPM to draw in sufficient airflow, it eventually crashes
it's a hard job to make a drone capable to fly into burning buildings
@JohnRennie Hi Sir! I was thinking, in formula for radial acceleration in polar coordinates, the term "r" in centripetal acceleration represents radius of curvature or radius vector (magnitude)?
I had this doubt when i was studying kepler's laws, while deriving velocity at apogee/perigee, I equated the force of gravity on a planet to centripetal acceleration (in which i used , mv^2/ r, where r is position vector at apogee/perigee from one of the foci and v is the velocity of planet at apogee/perigee. I didn't get the answer, in fact the answer used R(radius of curvature at apogee/perigee) instead of radius vector.
But i believe, when we write centripetal acceleration in polar coordinates, r is radius vector...
It's because the centripetal acceleration at apogee and perigee is not equal to the gravitational acceleration.
At apogee the centripetal acceleration is less than the gravitational acceleration, and that's why after the apogee the body falls inwards i.e. 𝑟 decreases.
At perigee the centripetal acceleration is greater than the gravitational acceleration, and that's why after the perigee the body moves outwards i.e. 𝑟 increases.
@JohnRennie umm..... sorry sir, but i didn't get it.... you say that radial acceleration = -GM/r² + v²/r, but shouldn't it be equal to gravitational acceleration???
But take a point to one side of the straight line and measure the 𝑟 coordinate from that point, then 𝑟 is not constant as the particle moves along the line. Yes?
The equation you posted above gives the acceleration vector i.e. the rate of change of the velocity vector. It's the acceleration you would feel (the "g force") if you were the one moving.
@JohnRennie i think I get this, I misunderstood d²r/dt² , it is in fact how radius vector's "magnitude" changes(like you said), but can we determine this? if we know say, distance of apogee/perigee and masses, other essential things(like semi major and minor axes,etc.) but not the velocity at the apogee and perigee... Thanks sir